哈馬契斯谷
地質
在以下影像中可見到哈馬契斯谷的兩側坡壁有許多沖溝。部分科學家認為這樣的地貌代表火星直到最近仍有少量液態水流過火星表面[1]。
圖集
參考資料
- Heldmann, J. and M. Mellon. Observations of Martian gullies and constraints on potential formation mechanisms. 2004. Icarus. 168: 285-304.
- 延伸閱讀
- Bleamaster, L, Crown, D. (PDF). Lunar and Planetary Science Conference. 2004 [2012-03-14]. (原始内容存档 (PDF)于2017-08-12).
- Price, K. . Lunar and Planetary Science Conference. 1992.
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